| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.92 | 336.08 | 28.28 | 194.40 | 27.85 | 44.44 | -19.92 | 35.75 | 0.5179 | -1056.7 | -388.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-11 09:58:58 UT
See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.55 | 0.00 | 0.87 | 28.02 | 49.68 | -14.68 | 28.05 | 0.4778 | -759.0 | -583.7 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 27.49 | 48.78 | -15.58 | 30.06 | 0.4776 | -808.0 | -554.2 | |
| 0.00 | 1.55 | 0.00 | 0.91 | 31.10 | 46.94 | -17.43 | 28.68 | 0.5364 | -608.0 | -532.6 | |
| 0.60 | 325.49 | 0.35 | 188.20 | 27.42 | 44.76 | -19.61 | 35.89 | 0.5102 | -1572.3 | -388.8 | |
| 45.22 | -4.00 | 26.13 | -4.00 | 27.81 | 44.47 | -19.89 | 35.76 | 0.5171 | -1250.7 | 999999 | |
| 3.10 | -4.00 | 1.80 | -4.00 | 28.23 | 44.10 | -20.26 | 35.70 | 0.5250 | -779.9 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.28 | 29.37 | 41.85 | -22.51 | 36.97 | 0.5570 | -253.0 | -315.5 | |
| 0.00 | 2.41 | 0.00 | 1.43 | 28.80 | 41.32 | -23.04 | 38.29 | 0.5557 | -846.0 | -664.5 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 25.91 | 37.74 | -26.62 | 45.95 | 0.5630 | 710.0 | 538.5 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 25.97 | 37.54 | -26.82 | 46.06 | 0.5656 | 433.0 | 434.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |